9โ€“13 Dec 2024
Kathmandu, Nepal
Asia/Kathmandu timezone

Session

Plenary

9 Dec 2024, 09:30
Kathmandu, Nepal

Kathmandu, Nepal

Conveners

Plenary: 1

  • Bibhushan Shakya (Deutsches Elektronen-Synchrotron (DE))

Plenary: 2

  • Anjan Giri

Plenary: 4

  • Suyog Shrestha (Washington College (US))

Plenary: 5

  • Anil Thapa (Colorado State University)

Plenary: 6

  • Sudip Jana (Max-Planck-Institut fรผr Kernphysik)

Plenary: 7

  • JESSICA TURNER

Plenary: 8

  • Brian Shuve (Harvey Mudd College)

Plenary: 9

  • Joseph Haley (Oklahoma State University (US))

Plenary: 10

  • Dr. Rukmani Mohanta

Plenary: 11

  • Niraj Dhital (Central Department of Physics, Tribhuvan University, Kathmandu, Nepal)

Plenary: 12

  • Bhupal Dev (Washington University in St. Louis)

Plenary: 13

  • Mu-Chun Chen (University of California - Irvine)

Plenary: 14

  • Michael Ratz

Presentation materials

There are no materials yet.

  1. Takaaki Kajita
    09/12/2024, 09:35
  2. Prof. Maxim Perelstein (Cornell University)
    09/12/2024, 10:10
  3. Harris Kagan (O), Harris Kagan (Ohio State University (US))
    09/12/2024, 11:05
  4. Bibhushan Shakya (Deutsches Elektronen-Synchrotron (DE))
    09/12/2024, 11:40
  5. Niraj Dhital
    09/12/2024, 12:05

    Physics and Society

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  6. Stefano Giagu (Sapienza Universitร  di Roma and INFN Roma (IT))
    10/12/2024, 09:00

    LHC Results: Experiment

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  7. Gagan Mohanty (Tata Institute of Fundamental Research (IN))
    10/12/2024, 09:35
  8. Amrit Gautam (The University of Kansas (US))
    10/12/2024, 10:10
  9. Michael Ratz
    10/12/2024, 11:05
  10. Prof. Mu-Chun Chen (University of California - Irvine)
    10/12/2024, 11:40
  11. Xiao-Gang He
    10/12/2024, 13:45
  12. Anjan Giri
    10/12/2024, 14:20

    Flavor Physics Theory

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  13. Dr. Rukmani Mohanta
    10/12/2024, 14:55
  14. Fernando Quevedo (The Abdus Salam International Centre for Theoretical Physics)
    11/12/2024, 09:00
  15. Amol Dighe (TIFR)
    11/12/2024, 09:35
  16. Marta Losada (NYUAD)
    11/12/2024, 10:10
  17. Joshua Ruderman (Princeton University)
    11/12/2024, 11:05
  18. Jan Heisig
    11/12/2024, 11:40

    The nature of dark matter poses one of the most pressing questions in fundamental physics today. While the thermal freeze-out of weakly interacting massive particles (WIMPs) has theoretical appeal, its validity is increasingly questioned due to experimental null results from colliders as well as direct and indirect detection experiments. In this talk, we explore dark matter genesis mechanisms...

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  19. Dr Alessandro Minotti (Universita & INFN, Milano-Bicocca (IT))
    12/12/2024, 09:00
  20. Mario Merola (University of Napoli Federico II and INFN - National Institute for Nuclear Physics)
    12/12/2024, 09:35
  21. Mohamed Rameez (Tata Institute of Fundamental Research)
    12/12/2024, 10:10

    Neutrino Experiment

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  22. Bhupal Dev (Washington University in St. Louis)
    12/12/2024, 11:05
  23. Giulia Ricciardi
    12/12/2024, 11:40
  24. Dr Sudip Jana (Max-Planck-Institut fรผr Kernphysik)
    12/12/2024, 13:45
  25. Prof. Sanjib Kumar Agarwalla (Institute of Physics, Bhubaneswar and University of Wisconsin-Madison)
    12/12/2024, 14:20
  26. Claire David (AIMS South Africa)
    12/12/2024, 14:55
  27. Francois BOUCHET
    13/12/2024, 09:00
  28. Daniel Tapia Takaki (University of Kansas)
    13/12/2024, 09:35
  29. Prolay Mal (National Institute of Science Education and Research (NISER) (IN))
    13/12/2024, 10:10
  30. Brian Shuve (Harvey Mudd College)
    13/12/2024, 11:05

    Hidden sectors can give rise to novel dynamics in the early universe, and correlated signatures in experiments today. I will discuss some examples of thermal and non-thermal hidden sectors that can account for dark matter and/or the baryon asymmetry, and present new results and prospects for experimental searches that improve our sensitivity to these hidden sectors.

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  31. JESSICA TURNER
    13/12/2024, 11:40
  32. Masahide Yamaguchi (Tokyo Institute of Technology)
    13/12/2024, 13:45
  33. Manjari Bagchi
    13/12/2024, 14:20

    Neutron stars are rapidly spinning, highly magnetised, extremely dense compact stars. They are believed to be composed of mostly neutrons and some amount of other baryons. There are even theories that free quarks exist near the core of neutron stars. Hence, knowing the properties of neutron stars observationally help us understand properties of matter at extreme densities. Neutron stars are...

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  34. Luciano Musa (CERN)
    13/12/2024, 14:55

    Physics and Society

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  35. Anil Thapa (University of Virginia)
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